Potential Neutrino Signals from Galactic -Ray Sources Alexander Kappes , Christian Stegmann University Erlangen-Nuremberg Felix Aharonian, Jim Hinton MPI für Kernphysik, Heidelberg TeV Particle Astrophysics II Madison WI, August 28 – 31, 2006 TeV -Ray Sources as Potential Sources From -Rays to Neutrinos Rates in a km 3 Neutrino Telescope
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Potential Neutrino Signals from Galactic -Ray Sources
Potential Neutrino Signals from Galactic -Ray Sources. Alexander Kappes , Christian Stegmann University Erlangen-Nuremberg Felix Aharonian, Jim Hinton MPI für Kernphysik, Heidelberg. TeV Particle Astrophysics II Madison WI, August 28 – 31, 2006. - PowerPoint PPT Presentation
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Potential Neutrino Signals from
Galactic -Ray Sources
Alexander Kappes, Christian StegmannUniversity Erlangen-Nuremberg
Felix Aharonian, Jim Hinton MPI für Kernphysik, Heidelberg
TeV Particle Astrophysics IIMadison WI, August 28 – 31, 2006
TeV -Ray Sources as Potential Sources From -Rays to Neutrinos Rates in a km3 Neutrino Telescope
TeV Particle Astrophysics II Madison WI, Aug. 28 - 31, 2006
2Alexander Kappes University Erlangen-Nuremberg
Introduction
How to derive neutrino flux from measured -ray flux?
What are the event rates in neutrino telescopes?
Most of our galaxy surveyed by TeV -ray detectors
Likely all bright Galactic TeV -ray sources identified
) neutrino source candidates
TeV Particle Astrophysics II Madison WI, Aug. 28 - 31, 2006
3Alexander Kappes University Erlangen-Nuremberg
Galactic TeV -Ray Sources (I)
7 Supernova Remnant (SNR) candidates Detection of resolved -ray emission from shells
RX J1713-3946 (H.E.S.S.) : Multiwavelength analysis points to hadronic origin
NCP: No counterpart at other wavelengths *no -ray absorption
20 further H.E.S.S. sources investigated: All -ray spectra show no cut-offs (but limited statistics) Event numbers mostly below 1 – 2 in 5 years For more details: preprint astro-ph/0607286
Sources with observed cut-off KM3NeT (1 km3, 5 years)
TeV Particle Astrophysics II Madison WI, Aug. 28 - 31, 2006
13Alexander Kappes University Erlangen-Nuremberg
Summary
Likely, strongest Galactic TeV -ray sources discovered
) neutrino source candidates
Measured -ray spectra allow robust prediction of neutrino fluxes
Simple relation between parameters of -ray and spectrum found
Event rates in a 1 km3 Mediterranean neutrino telescope (KM3NeT) about 1 event per year from each of brightest sources (E > 1 TeV)
about equal number of background and signal events